Project Longshot to Alpha Centauri - part 1

So I've started transcribing the scanned pdf of Project Longshot, a project planned in the 1980s devising a probe that would go to Alpha Centauri in the early 21st century, arriving after a 100-year flight. Actually about 70% of the pdf is legible enough that it can be copied and pasted, but the formulae and images of course don't register, and I'm enjoying learning about the project at the same time and uploading it here anyway.

NGT-21-002-080

NGT-80001

PROJECT LONGSHOT

AN UNMANNED PROBE TO ALPHA CENTAURI

U.S. NAVAL ACADEMY

NASA/USRA University Advanced Design

Program Project Report for 1987-1988

Keith A. Beals

Martin Beaulieu

Frank J. Dembia

Joseph Kerstiens

Daniel L. Kramer

Jeffrey R. West

James A. Zito

(NASA-CR-184718) PROJECT LONGSHOT: AN N89-16904

UNMANNED PROBE TO ALPHA CENTAURI Program

Project Report, 1987 – 1988 (Naval Academy)

74 p CSCL 22B Unclas

G3/18 0189673

PROJECT LONGSHOT

This report presents a preliminary design for an unmanned probe to Alpha Centauri with a planned launch early in the 21^st century. This mission was based upon a requirement stated in the report by the National Commission on Space, Pioneering the Space Frontier. The probe would be assembled at the space station and take approximately 100 years to reach the nearest star. Several technologies must be developed in order for this mission to be possible. A pulsed fusion microexplosion drive with 1,000,000 seconds of specific impulse is the primary enabling technology. A large, long-life fission reactor with 300 kilowatts power output is also required. Communications lasers would use 0.532 micron wavelength since there is minimal power output by the starts in that frequency band. A laser with an inupt power of 250 kilowatts would alow for a data rate of 1000 bits per second at maximum range. There are three types of information to be gathered by the probe: properties of the interstellar medium, characteristics of the three-star Alpha Centauri system, and astrometry (finding distances to starts using parallax measurements).

ACKNOWLEDGEMENTS

This project represents the United States Naval Academy participation in the NASA/USRA University Advanced Design Program. Seven first class midshipmen in the Aerospace Engineering Department (Astronautics track) performed this work in EA 439, Special Design (Fall semester 1987) and EA 470, Spacecraft Design (Spring semester 1988). The seven group members were Keith Beals, Martin Beaulieu, Frank Dembia, Joseph Kerstiens, Daniel Kramer, Jeffrey West, and James Zito.

The faculty advisors were Assistant Professor Walter K. Daniel and Professor George F. Pieper. The NASA representative from Goddard Space Flight Center was Dr. Stephen Paddack, who is also a Naval Academy Visiting Professor. Visiting Professor Fred Mobley from the John Hopkins Applied Physics Laboratory participated in the design courses.

1.0 MISSION MODEL

1.1 General Mission

The subject of this report is the design of an unmanned probe to Alpha Centauri. This mission is called for in the report by the National Commission on Space, Pioneering the Space Frontier. On pages 38 through 40 the commission outlines a program for solar and space physics which is planned for the period "beyond the initial operation of the space station," and includes "a long life high-velocity spacecraft to be sent out of the Solar System on a trajectory to the nearest star." Our probe will be a completely autonomous design based upon a combination of current technology and technological advances which can be reasonably expected to be developed over the next 20 to 30 years. The expected launch date is in the beginning of the next century with a transit time of 100 years.

The mission profile will be as follows:

1. Assembly of modular components on the ground.

2. Launch of components to LEO.

3. Assembly of components at Space Station.

4. Boost assembled and fueled spacecraft to injection point for interstellar trajectory using chemical upper stage.

5. Start main fusion drive and begin interstellar flight which will last approximately 100 years.

6. During this period will be returned on the interstellar medium and magnetic fields.

7. Enter elliptical orbit around Beta Centauri and begin transmission of data.

1.2 Technology

Using purely current technologies, a mission to another star system would be impossible to complete. There are basically three main areas where advances are needed: propulsion, data processing for command and control functions, and reliability.

In order to reduce transit time to an acceptable length, specific impulses on the order of 10E6 seconds are required. This represents an increase of several orders of magnitude over chemical rockets and nuclear rocket models which can be implemented using only present technology. To achieve the required levels of impulse, a pulsed fusion reactor based rocket engine is proposed. Based on the current level of technology in the field of microbomb fusion it is reasonable to assume that in 20 to 30 years such a system will be possible.

Due to the great distance at which the probe will operate, positive control from earch will be impossible due to the great time delays involved. This fact necessitates that the probe be able to think for itself. In order to accomplish this, advances will be required in two related but separate fields, artificial intelligence and computer hardware. IA research is advancing at a tremendous rate. Progress during the last decade has been phenomenal and there is no reason to expect it to slow any time soon.

Therefore, it should possible to design a system with the required intelligence by the time that this mission is expected to be launched. The problem with basing the design on current hardware is one of weight and speed. Producing a system with the required intelligence and speed, while including the needed redundancy using current technology, would result in a huge unit requiring a cooling system as large as a nuclear power plant's. Current advances have shrunk a Cray 2 from a room sized system needing a huge cooling plant to two chips, and with the advent of high temperature super-conductor technology there is every reason to assume that many more such quantum leaps in computer technology may be expected in the next 20 to 30 years.

Since no one has ever designed a dynamic system to last for more than a century, it is impossible to guess just how much the reliability of current systems will have to be improved. However, many satellites which were designed with mission lives of only a few years have operated for much longer periods of time, often failing merely because they ran out of expendables. The Transit family is a good example: they were designed to last for only 18 months and there are some still operating after 18 years or more. Other examples include Pioneer, Mariner, Voyager, and Viking. With successes in reliability such as these, and the improvements in simulation technology which will come with the improvements in computer technology (discussed in the previous paragraph), there should be no difficulty in designing in the required reliability.

1.3 Infrastructure

A very strong effort towards space exploration will be required to complete this mission and this commitment will have to begin in order to ensure that those systems essential for the production of the probe and its initial boost phase will be in place when the enabling technologies are realized. These systems include a heavy-lift launch vehicle, a large space station and an advanced, high energy upper stage. These requirements represent merely the technological infrastructure; also required is a very large initial human infrastructure, as well as a long term human commitment.

The heavy-lift launcher is needed since current weight estimates for the spacecraft are in excess of 350 metric tons. Even after taking into account the assumption that the ship will be launched to LEO as a series of modular components, the size ofmany of the modules precludes their launch on the Shuttle. Additionally, some units will be too massive and complex to be launched by available launch vehicles.

Since a basic assumption in this analysis is that the probe will be launched in a modular form and assembled in orbit, it is necessary to provide an orbiting base of operations for the personnel assembling the components of the spacecraft. This base will be the Space Station. Requirements for the station will include:

-Capability to house a large work force to include assemble technicians and test engineers.

-A number of large manipulator arms and sufficient mechanical support structure to allow attachment of all required assembly jigs.

-Adequate data processing capability to perform systems checks during assembly and thefinal system check-out following assembly.

Due to the nature of the main drive, it is both inadvisable and impossible to complete the mission by igniting the fusion drive in LEO. This fact leads to the requirement for the advanced upper stage. The planned in-solar system mission profile calls for a series of three burns using these upper stages to escape the solar system from which the interstellar injection may be made. This report will assume that the upper stage will have twice the impulse and similar weight characteristics to a Space Shuttle SRB.

The human side of the infrastructure will be a much greater challenge than the technical side because the required commitment spans such a long period of time. The time between the initial authorization for the mission until the return of the first data from the Alpha Centauri system will be well in excess of one century. In fact it will probably be on the order of two centuries when the time needed for hardware design, procurement, in-orbit assembly, and transit are considered. The effort required to design, build and launch the probe would be on the order of the Apollo project or much larger. The commitment at the other end of the mission should be an easy one to fulfill since scientists will be eager to analyze the incoming data. Thus, the greatest challenge coming with the caretaker portion of the mission - the century of travel time when very little data will be transmitted. The problem here is not the number of people required, since it will be small, but rather the time involved. There has never been a similar project in modern history carried out over such a long time scale. However, there have been organizations which have lasted for such a time. In fact, some have lasted longer! Some examples include: the militaries of nations such as the U.S. and U.K., various research institutions like the National Geographic Society and the Smithsonian Institution, and private organizations such as the Red Cross and the Explorer's Club. The precedent exists for organizations continuing for the required time frame. Therefore it can be assumed that the required support structure can be established.